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Energetic Gamma-Ray Event Telescope: Hard
These data are from the Compton GRO EGRET team. Data are from all pointings of the EGRET instrument in the verification phase and phase 1-4 of the Compton mission. The maps... -
Effelsberg-Bonn HI Survey
The Effelsberg-Bonn HI Survey (EBHIS) is a 21-cm survey performed with the 100-m telescope at Effelsberg. It covers the whole northern sky out to a redshift of z ~ 0.07 and... -
2nd Digitized Sky Survey (Blue)
The native projection of these data is described as a high-order polynomial distortion of a gnomonic projection using the same terms as the DSS. Provenance: Data taken by... -
First Digitized Sky Survey: Red Plates
This survey is the POSS1 Red plates from the original POSS survey. It covers the sky north of -30 degrees declination. Provenance: Data taken by CalTech Compression... -
First Digitized Sky Survey: Blue Plates
This survey uses the POSS1 Blue plates. Provenance: Data taken by CalTech, Compression and distribution by Space Telescope Science Institute.. This is a... -
Original Digitized Sky Survey
This survey comprises the compressed digitization of the Southern Sky Survey and the Palomar Sky Survey E plates as distributed on CD ROM by the Space Telescope Science... -
DRAO 22 MHz Survey
Roger et al. (1999) presented a map of the 22 MHz radio emission between declinations -28° and +80°, covering ~73% of the sky, derived from observations with the 22 MHz... -
CGRO Compton Telescope: 3 channel data
This survey is a maximum entropy solution to the data taken by the CompTel instrument on the Compton Gamma Ray Observatory. The data in this survey are intended only to give... -
Cosmic Background Explorer DIRBE Annual\ Average\ Map
The DIRBE Project Data Sets cover the whole sky and provide photometric data in 10 bands ranging in wavelength from 1.25 to 240 microns. SkyView has supported three maps: an... -
CO Galactic Plane Survey
New large-scale CO surveys of the first and second Galactic quadrants and the nearby molecular cloud complexes in Orion and Taurus, obtained with the Harvard-Smithsonian... -
JWST NEP TDF NuSTAR and XMM-Newton survey
We present the second NuSTAR and XMM-Newton extragalactic survey of the JWST North Ecliptic Pole (NEP) Time-Domain Field (TDF). The first NuSTAR NEP-TDF survey (Zhao et al.,... -
Ammonia observations of Planck cold cores
Single-pointing observations of NH_3_(1,1) and (2,2) were conducted toward 672 Planck Early Cold Cores (ECCs) using the Nanshan 26-m radio telescope. Out of these sources, a... -
HIPS Survey:CFHTLS W u
The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument... -
HIPS Survey:CFHTLS D u
The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument... -
LABOCA Extended Chandra Deep Field South Submillimetre Survey
The LABOCA Extended Chandra Deep Field South (ECDFS) Submillimetre Survey (LESS) is a public legacy survey of the ECDFS at 870 μm using the LABOCA camera (Siringo et al. 2009)... -
Swift BAT 70 Month All-Sky Survey: 14\-20 keV: flux
This BAT Hard X-ray Survey data is the 70-month survey product of the BAT instrument on the Swift observatory. Swift/BAT is a wide field-of-view (70x100 degrees) hard X-ray... -
AKARI N60
The AKARI (formerly Astro-F) mission is a Japanese second generation all-sky infrared survey mission. SkyView currently includes surveys from the four bands of the FIS... -
4850 MHz Survey - GB6/PMN
The 4850MHz data is a combination of data from three different surveys: Parkes-MIT-NRAO (PMN) Southern (-88°; to -37°; declination) and tropical surveys... -
HI All-Sky Continuum Survey
This survey is a mosaic of data taken at Jodrell Bank, Effelsberg and Parkes telescopes. The data was distributed in the NRAO Images from the Radio Sky CD ROM. Provenance:... -
Two Micron All Sky Survey (H-Band)
2MASS data were collected by uniformly scanning the entire sky in three near-infrared bands to detect and characterize point sources brighter than about 1 mJy in each band,...
